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000007304 0247_ $$2DOI$$a10.1103/PhysRevLett.102.244801
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000007304 084__ $$2WoS$$aPhysics, Multidisciplinary
000007304 1001_ $$0P:(DE-HGF)0$$aMorozov, V.S.$$b0
000007304 245__ $$aExperimental Test of a New Technique to Overcome Spin-Depolarizing Resonances
000007304 260__ $$aCollege Park, Md.$$bAPS$$c2009
000007304 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article
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000007304 440_0 $$04925$$aPhysical Review Letters$$v244801$$x0031-9007$$y102
000007304 500__ $$aWe thank the COSY staff for the successful operation of COSY with its injector cyclotron and polarized ion source. We are grateful to E. D. Courant, Ya. S. Derbenev, D. Eversheim, G. Fidecaro, W. Haeberli, H. Huang, Yu. F. Orlov, H. Rohdjea, T. Roser, H. Sato, W. Scobel, E. J. Stephenson, K. Ulbrich, K. Yonehara, and others for their help and advice. This research was supported by grants from the German BMBF Science Ministry, its FFE program at COSY, and the Helmholtz Association through funds provided to the virtual institute "Spin and strong QCD'' (VH-VI-231).
000007304 520__ $$aWe recently tested a new spin resonance crossing technique, Kondratenko Crossing (KC), by sweeping an rf-solenoid's frequency through an rf-induced spin resonance with both the KC and traditional fast crossing (FC) patterns. Using both rf bunched and unbunched 1.85 GeV/c polarized deuterons stored in COSY, we varied the parameters of both crossing patterns. Compared to FC with the same crossing speed, KC reduced the depolarization by measured factors of 4.7 +/- 0.3 and 19(-5)(+12) for unbunched and bunched beams, respectively. This clearly showed the large potential benefit of Kondratenko Crossing over fast crossing.
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000007304 7001_ $$0P:(DE-HGF)0$$aChao, A.W.$$b1
000007304 7001_ $$0P:(DE-HGF)0$$aKrisch, A.D.$$b2
000007304 7001_ $$0P:(DE-HGF)0$$aLeonova, M.A.$$b3
000007304 7001_ $$0P:(DE-HGF)0$$aRaymond, R.S.$$b4
000007304 7001_ $$0P:(DE-HGF)0$$aSivers, D.W.$$b5
000007304 7001_ $$0P:(DE-HGF)0$$aWong, V.K.$$b6
000007304 7001_ $$0P:(DE-Juel1)VDB64148$$aGarishvili, A.$$b7$$uFZJ
000007304 7001_ $$0P:(DE-Juel1)VDB5067$$aGebel, R.$$b8$$uFZJ
000007304 7001_ $$0P:(DE-Juel1)131234$$aLehrach, A.$$b9$$uFZJ
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000007304 7001_ $$0P:(DE-Juel1)131248$$aMaier, R.$$b11$$uFZJ
000007304 7001_ $$0P:(DE-Juel1)VDB1283$$aPrasuhn, D.$$b12$$uFZJ
000007304 7001_ $$0P:(DE-Juel1)VDB5270$$aStockhorst, H.$$b13$$uFZJ
000007304 7001_ $$0P:(DE-Juel1)VDB64503$$aWelsch, D.$$b14$$uFZJ
000007304 7001_ $$0P:(DE-HGF)0$$aHinterberger, F.$$b15
000007304 7001_ $$0P:(DE-HGF)0$$aKondratenko, A.M.$$b16
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000007304 8567_ $$uhttp://dx.doi.org/10.1103/PhysRevLett.102.244801
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